Research and establishment of the X-ray monochromator at the 100XF
The 100-m X-ray Test Facility (100XF) was developed according to the calibration requirement of the first X-ray astronomical satellite Insight -HXMT in china. After that, the 100XF has provided calibration services for other X-ray astronomical satellites. In order to test the energy response matrice...
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| creator | Hou, Dongjie Zhang, Yifan Zhu, Yuxuan Zhao, Zijian Zhang, Ziliang Yang, Xiongtao Ma, Jia Xu, He Chen, Yong Xu, Yupeng Wang, Yusa Liu, Congzhan |
| description | The 100-m X-ray Test Facility (100XF) was developed according to the calibration requirement of the first X-ray astronomical satellite
Insight
-HXMT in china. After that, the 100XF has provided calibration services for other X-ray astronomical satellites. In order to test the energy response matrices of space-borne detectors and to extend the capability of 100XF, a monochromator based on channel-cut crystals is developed. So far, 3.0-20.7 keV monochromatic X-rays have been realized successfully with Si(111) crystal. The monochromaticity (
Δ
E
FWHM
/E) is better than 0.6% @5.9 keV, the flux stability can reach 2.6% in about one hour. The energy stability is particularly good, the variation is 0.05% in about one hour. Further more, the beam spot spreads in the plane orthogonal to the rocking direction after a propagation of 100-meter, which is sufficient and useful for testing detectors with large sensitive area. In this paper, we present the research and establishment of the X-ray monochromator at the 100XF. |
| doi_str_mv | 10.1007/s10686-024-09941-z |
| format | Article |
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Insight
-HXMT in china. After that, the 100XF has provided calibration services for other X-ray astronomical satellites. In order to test the energy response matrices of space-borne detectors and to extend the capability of 100XF, a monochromator based on channel-cut crystals is developed. So far, 3.0-20.7 keV monochromatic X-rays have been realized successfully with Si(111) crystal. The monochromaticity (
Δ
E
FWHM
/E) is better than 0.6% @5.9 keV, the flux stability can reach 2.6% in about one hour. The energy stability is particularly good, the variation is 0.05% in about one hour. Further more, the beam spot spreads in the plane orthogonal to the rocking direction after a propagation of 100-meter, which is sufficient and useful for testing detectors with large sensitive area. In this paper, we present the research and establishment of the X-ray monochromator at the 100XF.</description><identifier>ISSN: 0922-6435</identifier><identifier>EISSN: 1572-9508</identifier><identifier>DOI: 10.1007/s10686-024-09941-z</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Astronomical satellites ; Astronomy ; Calibration ; Chemistry and Earth Sciences ; Computer Science ; Detectors ; Observations and Techniques ; Orthogonality ; Physics ; Physics and Astronomy ; Satellites ; Stability ; Statistics for Engineering ; Test facilities ; X-rays</subject><ispartof>Experimental astronomy, 2024-06, Vol.57 (3), Article 21</ispartof><rights>The Author(s), under exclusive licence to Springer Nature B.V. 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c270t-10f6e2c8df24e070e3845e7b1b321926d1eca3b17448d4ca8346514c2140cb63</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10686-024-09941-z$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10686-024-09941-z$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Hou, Dongjie</creatorcontrib><creatorcontrib>Zhang, Yifan</creatorcontrib><creatorcontrib>Zhu, Yuxuan</creatorcontrib><creatorcontrib>Zhao, Zijian</creatorcontrib><creatorcontrib>Zhang, Ziliang</creatorcontrib><creatorcontrib>Yang, Xiongtao</creatorcontrib><creatorcontrib>Ma, Jia</creatorcontrib><creatorcontrib>Xu, He</creatorcontrib><creatorcontrib>Chen, Yong</creatorcontrib><creatorcontrib>Xu, Yupeng</creatorcontrib><creatorcontrib>Wang, Yusa</creatorcontrib><creatorcontrib>Liu, Congzhan</creatorcontrib><title>Research and establishment of the X-ray monochromator at the 100XF</title><title>Experimental astronomy</title><addtitle>Exp Astron</addtitle><description>The 100-m X-ray Test Facility (100XF) was developed according to the calibration requirement of the first X-ray astronomical satellite
Insight
-HXMT in china. After that, the 100XF has provided calibration services for other X-ray astronomical satellites. In order to test the energy response matrices of space-borne detectors and to extend the capability of 100XF, a monochromator based on channel-cut crystals is developed. So far, 3.0-20.7 keV monochromatic X-rays have been realized successfully with Si(111) crystal. The monochromaticity (
Δ
E
FWHM
/E) is better than 0.6% @5.9 keV, the flux stability can reach 2.6% in about one hour. The energy stability is particularly good, the variation is 0.05% in about one hour. Further more, the beam spot spreads in the plane orthogonal to the rocking direction after a propagation of 100-meter, which is sufficient and useful for testing detectors with large sensitive area. In this paper, we present the research and establishment of the X-ray monochromator at the 100XF.</description><subject>Astronomical satellites</subject><subject>Astronomy</subject><subject>Calibration</subject><subject>Chemistry and Earth Sciences</subject><subject>Computer Science</subject><subject>Detectors</subject><subject>Observations and Techniques</subject><subject>Orthogonality</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Satellites</subject><subject>Stability</subject><subject>Statistics for Engineering</subject><subject>Test facilities</subject><subject>X-rays</subject><issn>0922-6435</issn><issn>1572-9508</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNp9kLtOwzAUhi0EEqXwAkyRmA3n-BInI1QUkCohoQ7dLMdxSKsmLnY6tE-PaZDYmM7w344-Qm4R7hFAPUSEvMgpMEGhLAXS4xmZoFSMlhKKczKBkjGaCy4vyVWMGwAolVQT8vThojPBtpnp68zFwVTbdWw71w-Zb7KhddmKBnPIOt972wbfmcGHzAwnKW2v5tfkojHb6G5-75Qs58_L2StdvL-8zR4X1DIFA0VocsdsUTdMOFDgeCGkUxVWnGHJ8hqdNbxCJURRC2sKLnKJwjIUYKucT8ndWLsL_mufPtUbvw99WtQcJC8AS47JxUaXDT7G4Bq9C-vOhING0D-o9IhKJ1T6hEofU4iPoZjM_acLf9X_pL4BYW9qlw</recordid><startdate>20240601</startdate><enddate>20240601</enddate><creator>Hou, Dongjie</creator><creator>Zhang, Yifan</creator><creator>Zhu, Yuxuan</creator><creator>Zhao, Zijian</creator><creator>Zhang, Ziliang</creator><creator>Yang, Xiongtao</creator><creator>Ma, Jia</creator><creator>Xu, He</creator><creator>Chen, Yong</creator><creator>Xu, Yupeng</creator><creator>Wang, Yusa</creator><creator>Liu, Congzhan</creator><general>Springer Netherlands</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20240601</creationdate><title>Research and establishment of the X-ray monochromator at the 100XF</title><author>Hou, Dongjie ; Zhang, Yifan ; Zhu, Yuxuan ; Zhao, Zijian ; Zhang, Ziliang ; Yang, Xiongtao ; Ma, Jia ; Xu, He ; Chen, Yong ; Xu, Yupeng ; Wang, Yusa ; Liu, Congzhan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c270t-10f6e2c8df24e070e3845e7b1b321926d1eca3b17448d4ca8346514c2140cb63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Astronomical satellites</topic><topic>Astronomy</topic><topic>Calibration</topic><topic>Chemistry and Earth Sciences</topic><topic>Computer Science</topic><topic>Detectors</topic><topic>Observations and Techniques</topic><topic>Orthogonality</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Satellites</topic><topic>Stability</topic><topic>Statistics for Engineering</topic><topic>Test facilities</topic><topic>X-rays</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hou, Dongjie</creatorcontrib><creatorcontrib>Zhang, Yifan</creatorcontrib><creatorcontrib>Zhu, Yuxuan</creatorcontrib><creatorcontrib>Zhao, Zijian</creatorcontrib><creatorcontrib>Zhang, Ziliang</creatorcontrib><creatorcontrib>Yang, Xiongtao</creatorcontrib><creatorcontrib>Ma, Jia</creatorcontrib><creatorcontrib>Xu, He</creatorcontrib><creatorcontrib>Chen, Yong</creatorcontrib><creatorcontrib>Xu, Yupeng</creatorcontrib><creatorcontrib>Wang, Yusa</creatorcontrib><creatorcontrib>Liu, Congzhan</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Experimental astronomy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hou, Dongjie</au><au>Zhang, Yifan</au><au>Zhu, Yuxuan</au><au>Zhao, Zijian</au><au>Zhang, Ziliang</au><au>Yang, Xiongtao</au><au>Ma, Jia</au><au>Xu, He</au><au>Chen, Yong</au><au>Xu, Yupeng</au><au>Wang, Yusa</au><au>Liu, Congzhan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Research and establishment of the X-ray monochromator at the 100XF</atitle><jtitle>Experimental astronomy</jtitle><stitle>Exp Astron</stitle><date>2024-06-01</date><risdate>2024</risdate><volume>57</volume><issue>3</issue><artnum>21</artnum><issn>0922-6435</issn><eissn>1572-9508</eissn><abstract>The 100-m X-ray Test Facility (100XF) was developed according to the calibration requirement of the first X-ray astronomical satellite
Insight
-HXMT in china. After that, the 100XF has provided calibration services for other X-ray astronomical satellites. In order to test the energy response matrices of space-borne detectors and to extend the capability of 100XF, a monochromator based on channel-cut crystals is developed. So far, 3.0-20.7 keV monochromatic X-rays have been realized successfully with Si(111) crystal. The monochromaticity (
Δ
E
FWHM
/E) is better than 0.6% @5.9 keV, the flux stability can reach 2.6% in about one hour. The energy stability is particularly good, the variation is 0.05% in about one hour. Further more, the beam spot spreads in the plane orthogonal to the rocking direction after a propagation of 100-meter, which is sufficient and useful for testing detectors with large sensitive area. In this paper, we present the research and establishment of the X-ray monochromator at the 100XF.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s10686-024-09941-z</doi></addata></record> |
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| subjects | Astronomical satellites Astronomy Calibration Chemistry and Earth Sciences Computer Science Detectors Observations and Techniques Orthogonality Physics Physics and Astronomy Satellites Stability Statistics for Engineering Test facilities X-rays |
| title | Research and establishment of the X-ray monochromator at the 100XF |
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